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- W4251620123 abstract "ABSTRACT: Supernovae of Types Ia, Ib, and II contribute, on average, 10 51 ergs of turbulent energy to the interstellar medium for each 2 M o of new heavy elements. This permits a dynamical extension of the homogeneous one-zone model (with constant IMF and instantaneous recycling) that is familiar from studies of galactic chemical evolution. Chemically possible scenarios predict current kinetic energy inputs ranging from 10 39 to 10 40 erg yr −1 per solar mass of interstellar gas. Dynamical studies might narrow this." @default.
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- W4251620123 date "1989-01-01" @default.
- W4251620123 modified "2023-09-27" @default.
- W4251620123 title "Contributions of Supernovae to the Chemical and Dynamical Evolution of the ISM" @default.
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- W4251620123 doi "https://doi.org/10.1017/s0252921100024350" @default.
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